Electron-positron annihilation and the cosmic X-ray background
Technical Report
·
OSTI ID:5705270
The possibility that the processes responsible for the cosmic X-ray background (CXB) would also produce an e(-)-e(+) annihilation feature is examined. Under the assumption that these proesses are thermal, the absence of a strong e(-)-e( ) annihilation feature places constraints on the compactness (L/R ratio) of these sources. Observations favor souces of small compactness ratio.
- Research Organization:
- National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center
- OSTI ID:
- 5705270
- Report Number(s):
- N-8327935
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640103* -- Astrophysics & Cosmology-- Quasi-Stellar
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANNIHILATION
ANTILEPTONS
ANTIMATTER
ANTIPARTICLES
BACKGROUND RADIATION
BASIC INTERACTIONS
BREMSSTRAHLUNG
COSMIC RADIATION
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC INTERACTIONS
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
INTERACTIONS
IONIZING RADIATIONS
LEPTONS
LUMINOSITY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
POSITRONS
RADIATIONS
X RADIATION
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANNIHILATION
ANTILEPTONS
ANTIMATTER
ANTIPARTICLES
BACKGROUND RADIATION
BASIC INTERACTIONS
BREMSSTRAHLUNG
COSMIC RADIATION
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
ELECTROMAGNETIC INTERACTIONS
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
INTERACTIONS
IONIZING RADIATIONS
LEPTONS
LUMINOSITY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
POSITRONS
RADIATIONS
X RADIATION